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Atmospheric impacts of the strongest known solar particle storm of 775 AD
Sporadic solar energetic particle (SEP) events affect the Earth’s atmosphere and environment, in particular leading to depletion of the protective ozone layer in the Earth’s atmosphere, and pose potential technological and even life hazards. The greatest SEP storm known for the last 11 millennia (th...
Autores principales: | , , , , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group
2017
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5368659/ https://www.ncbi.nlm.nih.gov/pubmed/28349934 http://dx.doi.org/10.1038/srep45257 |
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author | Sukhodolov, Timofei Usoskin, Ilya Rozanov, Eugene Asvestari, Eleanna Ball, William T. Curran, Mark A. J. Fischer, Hubertus Kovaltsov, Gennady Miyake, Fusa Peter, Thomas Plummer, Christopher Schmutz, Werner Severi, Mirko Traversi, Rita |
author_facet | Sukhodolov, Timofei Usoskin, Ilya Rozanov, Eugene Asvestari, Eleanna Ball, William T. Curran, Mark A. J. Fischer, Hubertus Kovaltsov, Gennady Miyake, Fusa Peter, Thomas Plummer, Christopher Schmutz, Werner Severi, Mirko Traversi, Rita |
author_sort | Sukhodolov, Timofei |
collection | PubMed |
description | Sporadic solar energetic particle (SEP) events affect the Earth’s atmosphere and environment, in particular leading to depletion of the protective ozone layer in the Earth’s atmosphere, and pose potential technological and even life hazards. The greatest SEP storm known for the last 11 millennia (the Holocene) occurred in 774–775 AD, serving as a likely worst-case scenario being 40–50 times stronger than any directly observed one. Here we present a systematic analysis of the impact such an extreme event can have on the Earth’s atmosphere. Using state-of-the-art cosmic ray cascade and chemistry-climate models, we successfully reproduce the observed variability of cosmogenic isotope (10)Be, around 775 AD, in four ice cores from Greenland and Antarctica, thereby validating the models in the assessment of this event. We add to prior conclusions that any nitrate deposition signal from SEP events remains too weak to be detected in ice cores by showing that, even for such an extreme solar storm and sub-annual data resolution, the nitrate deposition signal is indistinguishable from the seasonal cycle. We show that such a severe event is able to perturb the polar stratosphere for at least one year, leading to regional changes in the surface temperature during northern hemisphere winters. |
format | Online Article Text |
id | pubmed-5368659 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2017 |
publisher | Nature Publishing Group |
record_format | MEDLINE/PubMed |
spelling | pubmed-53686592017-03-30 Atmospheric impacts of the strongest known solar particle storm of 775 AD Sukhodolov, Timofei Usoskin, Ilya Rozanov, Eugene Asvestari, Eleanna Ball, William T. Curran, Mark A. J. Fischer, Hubertus Kovaltsov, Gennady Miyake, Fusa Peter, Thomas Plummer, Christopher Schmutz, Werner Severi, Mirko Traversi, Rita Sci Rep Article Sporadic solar energetic particle (SEP) events affect the Earth’s atmosphere and environment, in particular leading to depletion of the protective ozone layer in the Earth’s atmosphere, and pose potential technological and even life hazards. The greatest SEP storm known for the last 11 millennia (the Holocene) occurred in 774–775 AD, serving as a likely worst-case scenario being 40–50 times stronger than any directly observed one. Here we present a systematic analysis of the impact such an extreme event can have on the Earth’s atmosphere. Using state-of-the-art cosmic ray cascade and chemistry-climate models, we successfully reproduce the observed variability of cosmogenic isotope (10)Be, around 775 AD, in four ice cores from Greenland and Antarctica, thereby validating the models in the assessment of this event. We add to prior conclusions that any nitrate deposition signal from SEP events remains too weak to be detected in ice cores by showing that, even for such an extreme solar storm and sub-annual data resolution, the nitrate deposition signal is indistinguishable from the seasonal cycle. We show that such a severe event is able to perturb the polar stratosphere for at least one year, leading to regional changes in the surface temperature during northern hemisphere winters. Nature Publishing Group 2017-03-28 /pmc/articles/PMC5368659/ /pubmed/28349934 http://dx.doi.org/10.1038/srep45257 Text en Copyright © 2017, The Author(s) http://creativecommons.org/licenses/by/4.0/ This work is licensed under a Creative Commons Attribution 4.0 International License. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in the credit line; if the material is not included under the Creative Commons license, users will need to obtain permission from the license holder to reproduce the material. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/ |
spellingShingle | Article Sukhodolov, Timofei Usoskin, Ilya Rozanov, Eugene Asvestari, Eleanna Ball, William T. Curran, Mark A. J. Fischer, Hubertus Kovaltsov, Gennady Miyake, Fusa Peter, Thomas Plummer, Christopher Schmutz, Werner Severi, Mirko Traversi, Rita Atmospheric impacts of the strongest known solar particle storm of 775 AD |
title | Atmospheric impacts of the strongest known solar particle storm of 775 AD |
title_full | Atmospheric impacts of the strongest known solar particle storm of 775 AD |
title_fullStr | Atmospheric impacts of the strongest known solar particle storm of 775 AD |
title_full_unstemmed | Atmospheric impacts of the strongest known solar particle storm of 775 AD |
title_short | Atmospheric impacts of the strongest known solar particle storm of 775 AD |
title_sort | atmospheric impacts of the strongest known solar particle storm of 775 ad |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5368659/ https://www.ncbi.nlm.nih.gov/pubmed/28349934 http://dx.doi.org/10.1038/srep45257 |
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